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      On transient climate change at the Cretaceous−Paleogene boundary due to atmospheric soot injections

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          Significance

          A mass extinction occurred at the Cretaceous−Paleogene boundary coincident with the impact of a 10-km asteroid in the Yucatán peninsula. A worldwide layer of soot found at the boundary is consistent with global fires. Using a modern climate model, we explore the effects of this soot and find that it causes near-total darkness that shuts down photosynthesis, produces severe cooling at the surface and in the oceans, and leads to moistening and warming of the stratosphere that drives extreme ozone destruction. These conditions last for several years, would have caused a collapse of the global food chain, and would have contributed to the extinction of species that survived the immediate effects of the asteroid impact.

          Abstract

          Climate simulations that consider injection into the atmosphere of 15,000 Tg of soot, the amount estimated to be present at the Cretaceous−Paleogene boundary, produce what might have been one of the largest episodes of transient climate change in Earth history. The observed soot is believed to originate from global wildfires ignited after the impact of a 10-km-diameter asteroid on the Yucatán Peninsula 66 million y ago. Following injection into the atmosphere, the soot is heated by sunlight and lofted to great heights, resulting in a worldwide soot aerosol layer that lasts several years. As a result, little or no sunlight reaches the surface for over a year, such that photosynthesis is impossible and continents and oceans cool by as much as 28 °C and 11 °C, respectively. The absorption of light by the soot heats the upper atmosphere by hundreds of degrees. These high temperatures, together with a massive injection of water, which is a source of odd-hydrogen radicals, destroy the stratospheric ozone layer, such that Earth’s surface receives high doses of UV radiation for about a year once the soot clears, five years after the impact. Temperatures remain above freezing in the oceans, coastal areas, and parts of the Tropics, but photosynthesis is severely inhibited for the first 1 y to 2 y, and freezing temperatures persist at middle latitudes for 3 y to 4 y. Refugia from these effects would have been very limited. The transient climate perturbation ends abruptly as the stratosphere cools and becomes supersaturated, causing rapid dehydration that removes all remaining soot via wet deposition.

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          Most cited references46

          • Record: found
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          The Community Earth System Model: A Framework for Collaborative Research

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            Photosynthetic rates derived from satellite-based chlorophyll concentration

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              • Record: found
              • Abstract: not found
              • Article: not found

              MSIS-86 Thermospheric Model

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                Author and article information

                Journal
                Proc Natl Acad Sci U S A
                Proc. Natl. Acad. Sci. U.S.A
                pnas
                pnas
                PNAS
                Proceedings of the National Academy of Sciences of the United States of America
                National Academy of Sciences
                0027-8424
                1091-6490
                5 September 2017
                21 August 2017
                : 114
                : 36
                : E7415-E7424
                Affiliations
                [1] a Atmospheric Chemistry Observations & Modeling Laboratory, National Center for Atmospheric Research , Boulder, CO 80307;
                [2] bLaboratory for Atmospheric and Space Physics, Department of Atmospheric and Ocean Sciences, University of Colorado at Boulder , Boulder, CO 80303
                Author notes
                1To whom correspondence should be addressed. Email: bardeenc@ 123456ucar.edu .

                Edited by John H. Seinfeld, California Institute of Technology, Pasadena, CA, and approved July 17, 2017 (received for review May 30, 2017)

                Author contributions: C.G.B., R.R.G., and O.B.T. designed research; C.G.B. performed research; C.G.B., R.R.G., O.B.T., and A.J.C. analyzed data; and C.G.B., R.R.G., and O.B.T. wrote the paper.

                Author information
                http://orcid.org/0000-0002-5330-2788
                Article
                PMC5594694 PMC5594694 5594694 201708980
                10.1073/pnas.1708980114
                5594694
                28827324
                4d082c39-4f4e-4d95-8036-53504536ff78
                History
                Page count
                Pages: 10
                Funding
                Funded by: National Aeronautics and Space Administration (NASA) 100000104
                Award ID: NNX09AM83G
                Categories
                PNAS Plus
                Physical Sciences
                Earth, Atmospheric, and Planetary Sciences
                PNAS Plus

                asteroid impact,Cretaceous,Chicxulub,extinction,soot
                asteroid impact, Cretaceous, Chicxulub, extinction, soot

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